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C. Schoenaers

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1 paper

astro-ph2008

Spectroscopic Mode Identification in Slowly Pulsating Subdwarf-B Stars

C. Schoenaers, A. E. Lynas-Gray

Mode identification is crucial for an asteroseismological study of any significance. Contrarily to spectroscopic techniques, methods such as period-fitting and multi-colour photome…

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